Limits on the Variability ofGUsing Binary-Pulsar Data

Abstract
One of the few experimental handles on unified theories of gravity with other interactions comes from possible time variation of coupling constants over the Hubble time: H01(7.67×1011 yr1)1. We present a new theory-independent estimate (consistent with zero) of the time variation of Newton's gravitational constant derived from the timing of the binary pulsar PSR 1913+16: Ġ0G0=(1.0±2.3)×1011 yr1. We anticipate that this estimate will become sharper as more data are acquired.

This publication has 25 references indexed in Scilit: